Spectroscopic evidence of a new energy scale for superconductivity in H 3 S

• Published in: Nature physics 2017-09, Vol.13 (9), p.859
• Main Authors: Capitani, F, Langerome, B, Brubach, J-B, Roy, P, Drozdov, A, Eremets, M I, Nicol, E J, Carbotte, J P, Timusk, T
• Format: Article
• Language: English
• ISSN: 1745-2473
• DOI: 10.1038/nphys4156

The discovery of a superconducting phase in sulfur hydride under high pressure with a critical temperature above 200 K has provided fresh impetus to the search for superconductors at ever higher temperatures. Although this systems displays all the hallmarks of superconductivity, the mechanism through which it arises remains to be determined. Here we provide a first optical spectroscopy study of this superconductor. Experimental results for the optical reflectivity of H S, under hydrostatic pressure of 150 GPa, for several temperatures and over the range 60 to 600 meV of photon energies, are compared with theoretical calculations based on Eliashberg theory. Two significant features stand out: some remarkably strong infrared active phonons at around 160 meV, and a band with a depressed reflectance in the superconducting state in the region from 450 meV to 600 meV. In this energy range H3S becomes more reflecting with increasing temperature, a change that is traced to superconductivity originating from the electron-phonon interaction. The shape, magnitude, and energy dependence of this band at 150 K agrees with our calculations. This provides strong evidence of a conventional mechanism. However, the unusually strong optical phonon suggests a contribution of electronic degrees of freedom.